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  2. Hypergiant - Wikipedia

    en.wikipedia.org/wiki/Hypergiant

    The yellow hypergiants are thought to be generally post-red supergiant stars that have already lost most of their atmospheres and hydrogen. A few more stable high mass yellow supergiants with approximately the same luminosity are known and thought to be evolving towards the red supergiant phase, but these are rare as this is expected to be a ...

  3. Yellow hypergiant - Wikipedia

    en.wikipedia.org/wiki/Yellow_hypergiant

    The yellow hypergiant is an expected phase of evolution as the most luminous red supergiants evolve bluewards, but they may also represent a different sort of star. LBVs during eruption have such dense winds that they form a pseudo-photosphere which appears as a larger cooler star despite the underlying blue supergiant being largely unchanged.

  4. 6 different subtypes discovered for depression: How that may ...

    www.aol.com/6-different-subtypes-discovered...

    They note that about 30% of people with depression do not adequately respond to treatment. They say the subtypes may help identify potential treatment responses for things such as antidepressants ...

  5. List of star extremes - Wikipedia

    en.wikipedia.org/wiki/List_of_star_extremes

    Nearest red giant: Arcturus: 36.7 light-years (11.3 pc) Nearest supergiant: Canopus: 309 light-years (95 pc) While it is frequently described as a yellow supergiant, especially in evolutionary terms, [16] it is classified as a bright giant based on spectrum. [17] [16] List of nearest supergiants: Nearest hypergiant: μ Cephei (Herschel's Garnet ...

  6. Yellow hypergiant - en.wikipedia.org

    en.wikipedia.org/.../mobile-html/Yellow_hypergiant

    The term "hypergiant" was used as early as 1929, but not for the stars currently known as hypergiants. [1] Hypergiants are defined by their '0' luminosity class, and are higher in luminosity than the brightest supergiants of class Ia, [2] although they were not referred to as hypergiants until the late 1970s. [3]

  7. RW Cephei - Wikipedia

    en.wikipedia.org/wiki/RW_Cephei

    RW Cephei has been classified as a semi-regular variable star of type SRd, meaning that it is a slowly varying yellow giant or supergiant. The General Catalogue of Variable Stars cites a 1952 study giving a period of approximately 346 days, [ 35 ] [ 5 ] while other studies suggest different periods and certainly no strong periodicity.

  8. Red giant - Wikipedia

    en.wikipedia.org/wiki/Red_giant

    Red giants vary in the way by which they generate energy: most common red giants are stars on the red-giant branch (RGB) that are still fusing hydrogen into helium in a shell surrounding an inert helium core; red-clump stars in the cool half of the horizontal branch, fusing helium into carbon in their cores via the triple-alpha process

  9. V509 Cassiopeiae - Wikipedia

    en.wikipedia.org/wiki/V509_Cassiopeiae

    HR 8752 in comparison to other yellow hypergiants and luminous blue variables. Prior to 1973, HR 8752 was a cool yellow hypergiant with an early G spectral type. Following a dramatic shedding of its outer layers, it has now jumped to mid-A hypergiant and is not expected to return to its cool state.

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